Primordial scalar power spectrum from the hybrid approach in loop cosmologies
Bao-Fei Li, Javier Olmedo, Parampreet Singh, Anzhong Wang

TL;DR
This paper compares the primordial scalar power spectra in different loop quantum cosmology models using the hybrid approach, revealing significant differences in predictions, especially for mLQC-I, and highlighting the impact of underlying quantization methods.
Contribution
It introduces a detailed comparison of scalar power spectra in LQC, mLQC-I, and mLQC-II within the hybrid approach, emphasizing differences from the dressed metric approach.
Findings
The amplitude difference between LQC and mLQC-II is about 50% in certain regimes.
mLQC-I shows a suppressed power spectrum in the infrared, contrasting with the dressed metric results.
Differences between dressed and hybrid approaches are significant for mLQC-I, but not for LQC and mLQC-II.
Abstract
We compare the primordial scalar power spectra in the loop cosmological models using the effective dynamics of the hybrid approach to cosmological perturbations in which the background is loop quantized but the perturbations are Fock quantized. The three loop cosmological models under consideration are the standard LQC, the modified LQC-I (mLQC-I) and the modified LQC-II (mLQC-II) in the spatially flat Friedmann-Lema\^itre-Robertson-Walker (FLRW) universe with a Starobinsky potential. These models arise from different regularizations of the classical Hamiltonian constraint in the symmetry reduced spacetimes and aim to capture certain features of quantization in loop quantum gravity. When applying the techniques in the hybrid approach to mLQC-I/II, we find the effective Mukhanov-Sasaki equations take the same form as in LQC. The difference among the three models is encoded in the unique…
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